The existence of the structural anisotropy of the Jagiellonian field of the galaxies

The investigations of anisotropy in the orientations of galaxies

“…The statistically significant anisotropy for the galaxy groups and clus-ters orientations inside the cone of the Jagellonian field R ∼ 3000 Mpc is in the range 105-120 deg. [29]. It also should be noticed that Mandzhos et al [31,32], during the analysis of UGC [10] (north hemisphere) and ESO [11] (south hemisphere) galaxies, found that galaxies major axes are distributed anisotropically.…”

“…The evidence for the structural anisotropy of the small-large galaxy structures inside of the deep-field surveys likely for example the Jagellonian field [28], was presented in [29], where the method of the effective ellipse of inertness was applied [30]. The statistically significant anisotropy for the galaxy groups and clus-ters orientations inside the cone of the Jagellonian field R ∼ 3000 Mpc is in the range 105-120 deg.…”

Searching for (data on) Cracow astroplates

“…In particular, we will attempt to repeat the previous galaxy counts for the Jagiellonian Field missing plates (if rediscovered), or for the existing Jagiellonian Field archival scans (Vavilova & Flin ) (if irretrievably lost), using more modern algorithms. These results will be used to compare the mechanisms of galaxy grouping with other large‐scale structures of the Universe, including radio quasars or the dark matter field (Gregul et al ). Another scientific project we want to get involved in is searching for new asteroids on all the unscanned 20th century plates, combined with obtaining more precise orbital parameters for the already known asteroids (Eglitis et al ; Miskova & Vitek ).…”